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Disk Rotation Curves in Triaxial Potentials

Published online by Cambridge University Press:  04 August 2017

Ortwin E. Gerhard  and
Mario Vietri
Ortwin E. Gerhard
Affiliation:
Max-Planck-Institut für Astrophysik, Garching, West Germany
Mario Vietri
Affiliation:
Osservatorio Astrofisico, Firenze, Italy

Abstract

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The apparent rotation curve of cold gas in a triaxial potential often differs from that in an axisymmetric system in characteristic ways. The data argue for triaxial bulges in our Galaxy and several others.

Type
Posters
Information
Symposium - International Astronomical Union , Volume 127: Structure and Dynamics of Elliptical Galaxies , 1987 , pp. 399 - 400
Copyright
Copyright © Reidel 1987 

References

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